Ohmic dissipation of the magnetospheric current inside the star
converts the rotation energy into heat,
which is eventually radiated away.
No angular momentum
is lost in this process.
We have shown that
the Ohmic heating results in different angular velocities
between the surface and interior of the star.
Consequently the way
the magnetospheric current inside the star closes
is coupled with the angular momentum transfer in the star and accordingly cannot
be solved solely by Ohm's law, as erroneously
done in [1]}.
